The MUSE Ultra Deep Field (MUDF). I. Discovery of a group of Lyα nebulae associated with a bright z ≈ 3.23 quasar pair

We present first results from Multi Unit Spectroscopic Explorer (MUSE) observations at the Very Large Telescope in the MUSE Ultra Deep Field (MUDF), a approximate to 1.2 x 1.4 arcmin(2) region for which we are collecting approximate to 200 hours of integral field spectroscopy. The approximate to 40-h observation completed to date reveals the presence of a group of three Ly alpha nebulae associated with a bright quasar pair at z similar or equal to 3.23 with projected separation of approximate to 500 kpc. Two of the nebulae are physically associated with the quasars which are likely powering the Ly alpha emission, and extend for greater than or similar to 100 kpc at a surface brightness level of approximate to 6 x 10(-19) erg s(-1) cm(-2) arcsee(-2). A third smaller (approximate to 35kpc) nebula lies at a velocity offset of approximate to 1550 km s(-1). Despite their clustered nature, the two large nebulae have properties similar to those observed in isolated quasars and exhibit no sharp decline in flux at the current depth, suggesting an even more extended distribution of gas around the quasars. We interpret the shape and the alignment of the two brighter nebulae as suggestive of the presence of an extended structure connecting the two quasar host galaxies, as seen for massive galaxies forming within gas-rich filaments in cosmological simulations.